2. Potential reference evapo(trans)piration

Penman-Monteith equation

Reference values for potential evapotranspiration and evaporation are estimated using the Penman-Monteith equation (Supit et al., 1994, Supit & Van Der Goot, 2003).Specifically, the potential reference evapotranspiration rate [mm/day] for the reference vegetation canopy is computed as follows:

\[ET0 = \frac{\Delta R_{na} + \gamma EA}{\Delta + \gamma}\]

where
    $ET0$:   is the potential evapotranspiration rate from reference vegetation canopy (closed vegetation canopy) $[\frac{mm}{day}]$
    $R_{na}$:   is the net absorbed radiation for the reference vegetation canopy $[\frac{mm}{day}]$
    $EA$:   is the evaporative demand of the reference vegetation canopy $[\frac{mm}{day}]$
    $\Delta$:   is the slope of the saturation vapour pressure curve $[\frac{mbar}{^\circ C}]$
    $\gamma$:   is the psychrometric constant $[\frac{mbar}{^\circ C}]$

The same equation is also used to estimate the potential evaporation from a water surface and the evaporation from a (wet) bare soil surface. This purpose is achieved by using different values for the net absorbed radiation term and for the evaporative demand.

The potential evaporation rate from a bare soil surface [mm/day] is then estimated by:

\[ES0 = \frac{\Delta R_{na,s} + \gamma EA_s}{\Delta + \gamma}\]

Finally, the potential evaporation rate from water surface [mm/day] is computed as follows:

\[EW0 = \frac{\Delta R_{na,w} + \gamma EA_w}{\Delta + \gamma}\]

where $R_{na,s}$ and $R_{na,w}$ are the net absorbed radiation of bare soil surface and the net absorbed radiation of water surface, respectively ($[\frac{mm}{day}]$); $EA_s$ and $EA_w$ are the evaporative demand of bare soil surface and the evaporative demand of water surface, respectively ($[\frac{mm}{day}]$).

The procedure to calculate potential evapo(transpi)ration is summarised in the following Figure.

img

Figure: Overview of procedure to calculate potential reference evapo(transpi)ration. Terms with an asterisk (*) are calculated separately for a reference vegetation canopy, a bare soil surface and an open water surface, respectively.

The table below lists the properties of the reference surfaces that are used in the computation of $ET0$, $ES0$ and $EW0$, respectively.

  α (surface albedo) fc (empirical constant in evaporative demand equation)
$ET0$ 0.23 1
$ES0$ 0.15 0.75
$EW0$ 0.05 0.5

Calculating net absorbed radiation

Calculating the net absorbed radiation term involves the following two steps:

  1. Calculate the Angot radiation (daily extra-terrestrial radiation)
  2. Calculate the net absorbed radiation

Some data sets (e.g. ERA5) provide pre-calculated values for both incoming solar radiation and net long-wave radiation. When both the datasets are available, LISVAP offers the possibility to use these values directly. Conversely, LISVAP applies the following protocol to compute the Angot radiaton.

Step 1: Angot radiation (daily extra-terrestrial radiation)

The daily extra-terrestrial radiation is the product of the solar constant at the top of the atmosphere and the integral of the solar height over the day:

\[R_{a,d} = S_{c, d} \int sin \ \beta \ dt_h\]

where
    $R_{a,d}$:   Daily extra-terrestrial radiation $[{\frac{J}{m^2 \ day}}]$
    $S_{c,d}$:   Solar constant at the top of the atmosphere $[{\frac{J}{m^2 \ s}}]$
    $\int sin \ \beta \ dt_h$:   Integral of the solar height over the day $[s]$


The solar constant on a given day is calculated as:

\[S_{c, d} = S_c(1 + 0.033 \cos[\frac{360 \ t_d}{365}])\]

where
    $S_c$:   Average solar radiation at the top of the atmosphere $[{\frac{J}{m^2 \ s}}]$ (= 1370 ${\frac{J}{m^2 \ s}}$)
    $S_{c,d}$:   Solar constant at the top of the atmosphere $[{\frac{J}{m^2 \ s}}]$
    $t_d$:   Calendar day number (1st of January is 1, etcetera) $[-]$


The calendar day number is always a number between 1 and 365.25 (taking into account leap years, a year has on average 365.25 days).


The integral of the solar height equals:

\[\int sin \beta \ dt_h = \begin{cases} 3600(L_d \cdot sin \ \delta \cdot sin \ \lambda) &[B_{ld} > 1]\\ 3600(L_d \cdot sin \ \delta \cdot sin \ \lambda + \frac{24}{\pi} \cdot cos \ \delta \cdot cos \ \lambda \cdot \sqrt{1-(tan \ \delta \cdot tan \ \lambda)^2}) &[B_{ld} \le 1] \end{cases}\]

where
    $L_d$:   Astronomical day length $[h]$
    $\delta$:   Solar declination $[^\circ]$
    $\lambda$:   Latitude $[^\circ]$

with:

\[B_{ld} = \frac{-sin (\frac{PD}{\pi})+sin \ \delta \cdot sin \ \lambda}{cos \ \delta \cdot \ cos \ \lambda}\]

where PD is a correction constant (-2.65).


The solar declination is a simple function of the calendar day number (td):

\[\delta = -23.45 \cdot cos[\frac{360(t_d + 10)}{365}]\]


The day length is given by:

\[\begin{cases} L_d = 24 &[B_{ld} > 1]\\ L_d = 12+ \frac{24}{180} \alpha sin(B_{ld}) &[0 \le B_{ld} \le 1]\\ L_d = 12+ \frac{24}{180} [\alpha sin(B_{ld}) - 360] & [B_{ld} < 0]\end{cases}\]

Step 2: Net absorbed radiation

The net absorbed radiation is calculated for three reference surfaces:

  1. Reference vegetation canopy
  2. Bare soil surface
  3. Open water surface

The following equation is used to calculate the net long-wave radiation[1] (Maidment, 1993):

\[R_{nl}= f \epsilon \sigma (T_{av}+273)^4\]

where
    $R_{nl}$:   Net long-wave radiation $[{\frac{J}{m^2 \ day}}]$
    $\sigma$:   Stefan Boltzmann constant: $4.903 \cdot 10^{-3}[{\frac{J}{m^2 \ K^4 \ day}}]$
    $f$:   Adjustment factor for cloud cover
    $\epsilon$:   Net emissivity between the atmosphere and the ground

The net emissivity is calculated as:

\[\epsilon = 0.56 - 0.079 \sqrt{e_a}\]

where
    $e_a$:   Actual vapour pressure $[mbar]$

The actual vapour pressure ea can be provided as input data or computed as a function of the surface pressure and of the near-surface specific humidity:

\[e_a = \frac{( P_{surf} \cdot Q_{air} )}{62.2}\]

where
    $P_{surf}$:   instantaneous sea level pressure $[pa]$
    $Q_{air}$:   2 m instantaneous specific humidity [-]

Alternatively, when the weather stations provide the dew point temperature $T_{dew}$, the actual vapour pressure can be computed using the Goudriaan formula (1977):

\[e_a= 6.10588 \cdot e^{\frac{17.32491 \cdot T_{dew}}{T_{dew}+238.102}}\]

The equation of Allen (1994) is used to estimate the cloud cover factor:

\[f= (1.8 \cdot Trans_{Atm} - 0.35)\]

where
    $f$:   Cloud cover adjustment factor [-] in between [0,1]
    $Trans_{Atm}$:   Atmospheric transition [-]

\[Trans_{Atm}=\frac{R_{g,d}}{R_{so}}\]

where $R_{g,d}$ is the daily-extra terrestrial radiation or the downward short wave radiation $R_{d,s}$, depending on the meteo set available. $R_{so}$ is a function of the Angot Radiation $R_{a,d}$ and of the altitude $z$ (given by the Digital Elevation Model):

\[R_{so}= R_{a,d} \cdot (0.75 + ( 2 \cdot 10^5 \cdot z))\]

Finally, the net absorbed radiation [mm day-1] is calculated as:

\[R_{na}=\frac{(1- \alpha)R_{g,d}-R_{nl}}{L}\]

where
    $\alpha$:   Albedo (reflection coefficient) of the surface, the values are: $\alpha=0.23$ for the reference vegetation canopy, $\alpha=0.15$ for bare soil surface, and $\alpha=0.05$ for an open water surface (as indicated in the table at the beginning of this page)
    $R_{g,d}$:   Daily-extra terrestrial radiation or downward short wave radiation $R_{d,s}$ (depending on the available dataset)
    $R_{nl}$:   Net long-wave radiation
    $L$:   Latent heat of vaporization $[\frac{MJ}{kg}]$

$L$ is computed as follows:

\[L=2.501-2.361 \cdot 10^{-3} \cdot T_{av}\]

The net absorbed radiation is calculated for three cases: the reference vegetation canopy ($\alpha=0.23$), a bare soil surface ($\alpha=0.15$), and an open water surface ($\alpha=0.05$).

Evaporative demand of the atmosphere

The evaporative demand of the atmosphere is calculated as:

\[EA= 0.26(e_s-e_a)(f_c+BU \cdot u(2))\]

where
    $EA$:   Evaporative demand $[\frac{mm}{day}]$
    $e_s$:   Saturated vapour pressure $[mbar]$
    $e_a$:   Actual vapour pressure $[mbar]$
    $f_c$:   Empirical constant $[-]$, the values are $fc =1.0$ for the reference vegetation canopy, $fc =0.75$ for a bare soil surface, and $fc =0.5$ for an open water surface (as indicated in the table at the beginning of this page)
    $BU$:   Coefficient in wind function $[-]$
    $u(2)$:   Mean wind speed at 2 m height $[\frac{m}{s}]$

The Saturated vapour pressure is calculated as a function of mean daily air temperature:

\[e_s= 6.10588 \cdot e^{\frac{17.32491 \cdot T_{av}}{T_{av}+238.102}}\]

The coefficient in the wind function, $BU$, also depends on the temperature:

\[BU=max[0.54+0.35 \frac{\Delta T-12}{4}, 0.54]\]

Here, $\Delta T$ is the difference between the daily maximum and minimum temperature. The equation implies that $BU$ has a fixed value of 0.54 if $\Delta T$ is less than 12°C.

Since wind speed is usually measured at a height of 10 m, the following correction is made (Maidment (1993), p. 4.36):

\[u(2)=0.749 \cdot u(10)\]

where $u(10)$ is the measured wind speed at 10 m height $[\frac{m}{s}]$.

Similar to the calculation of the net absorbed radiation, the evaporative demand is calculated for three cases: for a reference vegetation canopy (using $fc =1.0$), a bare soil surface ($fc =0.75$), and an open water surface ($fc =0.5$).

Psychrometric constant

The psychrometric constant at sea level can be calculated as:

\[\gamma_0 = 0.00163 \frac{P_0}{L}\]

where
    $\gamma_0$:   Psychrometric constant at sea level (about 0.67) $[\frac{mbar}{^\circ C}]$
    $P_0$:   Atmospheric pressure at sea level $[mbar]$
    $L$:   Latent heat of vaporization $[\frac{MJ}{kg}]$

Since the barometric pressure changes with altitude, so does the psychrometric constant. The following altitude correction is applied (Allen et al., 1998):

\[\gamma(z)= \gamma_0(\frac{293-0.0065 \cdot z}{293})^{5.26}\]

where
    $\gamma(z)$:   Psychrometric constant at altitude z $[\frac{mbar}{^\circ C}]$
    $z$:   Altitude above sea level $[m]$

Slope of the saturation vapour pressure curve

The slope of the saturation vapour pressure curve is calculated as follows:

\[\Delta=\frac{238.102 \cdot 17.32491 \cdot e_s}{(T+238.102)^2}\]

where $\Delta$ is in $[\frac{mbar}{^\circ C}]$.

Potential evapo(transpi)ration

As explained before, potential evapo(transpi)ration is calculated for three reference surfaces:

  1. A closed canopy of some reference crop ($ET0$)
  2. A bare soil surface ($ES0$)
  3. An open water surface ($EW0$)

These quantities are all calculated using the Penman-Monteith equation, but using different values for the net absorbed radiation (Rna) and evaporative demand (EA):

\[ET0 = \frac{\Delta R_{na}+\gamma EA}{\Delta + \gamma}\] \[ES0 = \frac{\Delta R_{na,s}+\gamma EA_s}{\Delta + \gamma}\] \[EW0 = \frac{\Delta R_{na,w}+\gamma EA_w}{\Delta + \gamma}\]

where
    $ET0$:   Potential evapotranspiration for reference crop $[\frac{mm}{day}]$
    $ES0$:   Potential evaporation for bare soil surface $[\frac{mm}{day}]​$
    $EW0$:   Potential evaporation for open water surface $[\frac{mm}{day}]$
    $R_{na}$:   Net absorbed radiation, reference crop $[\frac{mm}{day}]$
    $R_{na,s}$:   Net absorbed radiation, bare soil surface $[\frac{mm}{day}]$
    $R_na,w$:   Net absorbed radiation, open water surface $[\frac{mm}{day}]$
    $EA$:   Evaporative demand, reference crop $[\frac{mm}{day}]$
    $EA_s$:   Evaporative demand, bare soil surface $[\frac{mm}{day}]$
    $EA_w$:   Evaporative demand, open water surface $[\frac{mm}{day}]$
    $\Delta$:   Slope of the saturation vapour pressure curve $[\frac{mbar}{^\circ C}]$
    $\gamma$:   Psychrometric constant $[\frac{mbar}{^\circ C}]$


[1] Note that this term is mistakenly called ‘net outgoing longwave radiation’ in the WODOST/CGMS documentation (Supit et. al.,2003), whereas it is in fact the net longwave radiation